Light Source Modules for Noise Mitigation

ABSTRACT

Configurations for light source modules and methods for mitigating coherent noise are disclosed. The light source modules may include multiple light source sets, each of which may include multiple light sources. The light emitted by the light sources may be different wavelengths or the same wavelength depending on whether the light source module is providing redundancy of light sources, increased power, coherent noise mitigation, and/or detector mitigation. In some examples, the light source may emit light to a coupler or a multiplexer, which may then be transmitted to one or more multiplexers. In some examples, the light source modules provide one light output and in other examples, the light source modules provide two light outputs. The light source modules may provide light with approximately zero loss and the wavelengths of light may be close enough to spectroscopically equivalent respect to a sample and far enough apart to provide coherent noise mitigation.

CROSS-REFERENCE TO RELATED APPLICATIONS

This application claims the benefit under 35 U.S.C. § 119(e) of U.S.Provisional Patent Application No. 63/219,483, filed Jul. 8, 2021, thecontents of which are incorporated herein by reference in theirentirety.

FIELD

This disclosure relates generally to optical measurement systems with alight source module. More particularly, this disclosure relates to alight source module including multiple light sources that providecoherent noise mitigation for spectroscopic measurements.

BACKGROUND

Generally, coherent noise is a noise source in various types of imagingsystems and may cause unwanted modifications of a signal. Coherent noisemay degrade images in optical systems designed to measure spectroscopicinformation of a sample. Coherent noise may cause graininess, granularpatterns, or intensity patterns in the measured signal or image. In someexamples, this type of noise may significantly interfere with theinformation content of an optical signal. Some known systems may producesignals with so much coherent noise that it may be difficult todetermine spectroscopic information in a corresponding measured signal.Thus, an optical measurement system that can mitigate coherent noise maybe desired.

SUMMARY

Embodiments of the systems, devices, methods, and apparatuses describedin the present disclosure are directed optical measurement systems andlight source modules for use in these systems. Also described aresystems, devices, methods, and apparatuses directed to providingde-cohered light that is spectroscopically equivalent with respect to agiven measurement. The optical system may include multiple light sourcesthat provide de-cohered light via phase shifts, different wavelengths,and so forth. The light source module may output one or more wavelengthsof light, and may provide functionality to address issues relating toredundancy, increased power to effectively reduce detector noise, and/orcoherent noise mitigation.

In some examples, the present disclosure describes a method of that mayinclude emitting a first light output having a first wavelength,emitting a second light output having a second wavelength, and combiningthe first light output and the second light output into a combined lightoutput having the first wavelength and the second wavelength. The methodmay further include receiving a portion of the combined light output atan optical detector, the portion of the combined light output returnedfrom the sample, and determining spectroscopic information for thesample from the portion of the combined light output. The first andsecond light outputs produce a coherent noise at the sample, thecoherent noise having a coherent noise bandwidth, and the spectroscopicinformation has a spectroscopic information bandwidth. The firstwavelength and the second wavelength are separated by an interstitialrange that is less than the spectroscopic information bandwidth and thatis greater than the coherent noise bandwidth.

In some of these variations, the first light output is infrared lightand the second light output is infrared light. Additionally oralternatively, the interstitial range is less than four nanometers. Insome variations, the interstitial range is between one and fournanometers. In some instances, the first light output is emitted from alight emitter, the operation of determining spectroscopic informationfor the sample is performed by a processing unit, and the light emitter,the optical detector, and the processing unit are all within a housing.The coherent noise bandwidth may include a range of wavelengths withinwhich two or more spectroscopic measurements of the sample have an rvalue that is greater than 0.5. In some of these coherent noisebandwidth is approximately one nanometer.

Other embodiments described here include a light source module having afirst semiconductor light source operative to emit a first wavelength oflight and a second semiconductor light source operative to emit a secondwavelength of light that is different than the first wavelength oflight. The light source module also includes a first optical junctionoperative to provide a first light output that includes the first andsecond wavelengths of light, a second optical junction operative toprovide a second light output that includes the first and secondwavelengths of light, and a multiplexer operative to provide a combinedlight output, such that the first wavelength of light provides a firstcoherent noise view and the second wavelength of light provides a secondcoherent noise view, thereby mitigating coherent noise.

In some of these variations, the first and second optical junctions arewavelength dependent multiplexers, each of the first and secondwavelengths of light are within four nanometers of each other such thateach of the first and second wavelengths of light are spectroscopicallyequivalent to one another. The light sources may act as redundantsemiconductor light sources, and may be used together to provideincreased power. Additionally or alternatively, each of the first andsecond wavelengths of light are spaced apart so that each wavelength oflight provides a different coherent noise view, thereby mitigatingcoherent noise. In some instances, the first optical junction is a firstMach-Zehnder interferometer, and the second optical junction is a secondMach-Zehnder interferometer. In some instances, the first opticaljunction is operative to select one of the first or second wavelengthsof light to output first output light, and the second optical junctionis operative to select one of third or fourth wavelengths of light tooutput second output light. Each of the first and second wavelengths oflight may spectroscopically equivalent to each other.

Still other embodiments described herein include a light source modulehaving a first set of semiconductor light sources operative to emit afirst set of wavelengths of light and a second set of semiconductorlight sources operative to emit a second set of wavelengths of light.The light source module also includes a first wavelength independentcoupler operative to output a first combined output derived from thefirst and second sets of wavelengths of light, and a second combinedoutput derived from the first and second sets of wavelengths of light.The light source module further includes a second wavelength independentcoupler operative to output a third combined output derived from thefirst and second sets of wavelengths of light and a fourth combinedoutput derived from the first and second sets of wavelengths of light.

A first multiplexer is operative to receive the first combined output,receive the second combined output, output a first half of the firstcombined output, and output a first half of the second combined output.A second multiplexer is operative to receive the first combined output,receive the second combined output, output a second half of the firstcombined output, and output a second half of the second combined output.The first, second, third, and fourth combined outputs may be derivedfrom different combinations of the first and second sets of wavelengthsof light, the first set of wavelengths of light may provide a first setof coherent noise views, the second set of wavelengths of light mayprovide a second set of coherent noise views, and the first and secondsets of coherent noise views mitigate coherent noise.

In some of these variations, the light source module includes a firstwaveguide coupled between the first wavelength independent coupler andthe first multiplexer and a second waveguide coupled between the firstwavelength independent coupler and the second multiplexer. The lightsource module further includes a third waveguide coupled between thesecond wavelength independent coupler and the first multiplexer, and afourth waveguide coupled between the second wavelength independentcoupler and the second multiplexer. In some instances, at least twowaveguides of the first, second, third, and fourth waveguides crosspaths with one another. Additionally or alternatively, each of the firstand second sets of wavelengths of light are within four nanometers ofeach other and are spectroscopically equivalent, and each of the firstand second sets of wavelengths of light is each greater than onenanometer apart from a closest wavelength of light to provide coherentnoise mitigation.

In other variations, the first half of the first combined output istransmitted to a first launch region, and the second half of the firstcombined output by the second multiplexer is transmitted to a secondlaunch region. Additionally or alternatively, the light source modulemay include a first waveguide coupled between the first wavelengthindependent coupler and the first multiplexer, a second waveguidecoupled between the first wavelength independent coupler and the secondmultiplexer, a third waveguide coupled between the second wavelengthindependent coupler and the first multiplexer, and a fourth waveguidecoupled between the second wavelength independent coupler and the secondmultiplexer, wherein none of the first, second, third, and fourthwaveguides crosses paths with one another. In some variations, the firstand second multiplexers are Echelle gratings. Each of the first andsecond sets of wavelengths of light may be spectroscopically equivalentto one another. In some variations, the first wavelength independentcoupler is a two by two multimode interferometer, and the secondwavelength independent coupler is a two by two multimode interferometer.

Still other embodiments are direct to methods for performing aspectroscopic measurement of a sample. These methods may includeperforming a set of measurements to generate multiple sets of measuredsignals and generating spectroscopic information using the multiple setsof measured signals. The set of measurements may include a first seriesof measurements and each measurement of the first series of measurementshas a corresponding pair of spectroscopically equivalent wavelengths.Each measurement of the first series of measurements includes emittinglight at the corresponding pair of spectroscopically equivalentwavelengths to the sample, and measuring light returned from the sampleto generate a set of measured signals of the multiple sets of measuredsignals.

In some instances, emitting light at the corresponding pair ofspectroscopically equivalent wavelengths includes simultaneouslygenerating light of a first wavelength of the corresponding pair ofspectroscopically equivalent wavelengths using a first light source andgenerating light of a second wavelength of the corresponding pair ofspectroscopically equivalent wavelengths using a second light source.Additionally or alternatively, the set of measurements includes a secondseries of measurements, each of which includes emitting light at thecorresponding wavelength to the sample and measuring light returned fromthe sample to generate a set of measured signals of the multiple sets ofmeasured signals. In some of these variations, at least one measurementin the first series of measurements is performed simultaneously with atleast one measurement in the second series of measurements.

In other instances, the method includes determining whether a firstlight source configured to generate a first wavelength meets a first setof operating criteria, and determining whether a second light sourceconfigured to generate a second wavelength meets a second set ofoperating criteria. The method may include performing, in response todetermining that both the first light source meets the first set ofoperating criteria, and the second light source meets the second set ofoperating criteria, a measurement of the first series of measurementsusing the first wavelength and the second wavelength as thecorresponding pair of spectroscopically equivalent wavelengths. Themethod may include performing, in response to determining that the firstlight source meets the first set of operating criteria and the secondlight source does not meet the second set of operating criteria, ameasurement of the second series of measurement using the firstwavelength as the corresponding wavelength. In some variations, thecorresponding pair of spectroscopically equivalent wavelengths for eachmeasurement of the first series of measurement provides differentcoherent noise views.

Other embodiments described herein are directed to a light source modulehaving a plurality of pairs of light sources that collectively form aset of paired light sources having a first light source subset and asecond light source subset, wherein each of the plurality of pairs oflight sources includes a first light source configured to output lightat a corresponding first wavelength, the first light source being partof the first light source subset, and a second light source configuredto output light at a corresponding second wavelength separated by lessthan a target separation amount, the second light source being part ofthe second light source subset. The light source module further includesa first multiplexer optically connected to the first light source subsetand configured to multiplex light received from the first light sourcesubset, a second multiplexer optically connected to the first lightsource subset and configured to multiplex light received from the secondlight source subset, and a multiplexing unit configured to opticallyconnect an output of the first multiplexer and an output of the secondmultiplexer to the set of outputs.

In some instances, the target separation amount may be 5 nanometers.Additionally or alternatively, the corresponding first wavelength andthe corresponding second wavelength for each of the plurality of pairsof light sources are separated by at least 1 nanometer. In somevariations, the light source module further includes a set of additionallight sources and a third multiplexer optically connected to the set ofadditional light sources and configured to multiplex light received fromthe second light source subset, such that the multiplexing unit isconfigured to optically connect an output of the third multiplexer tothe set of outputs. In some of these variations, each of the additionallight sources is configured to output a corresponding wavelength that isseparated from each the corresponding first and second wavelengths ofeach of the plurality of pairs of light sources by at least the targetseparation amount.

Another embodiment described herein includes an optical measurementsystem that includes a controller and a light source module having a setof outputs. The light source module may include a plurality of sets oflight sources including a first set of light sources and a second set oflight sources, a plurality of wavelength-specific multiplexers, each ofwhich has an output and is configured to multiplex a corresponding setof light sources of the plurality of sets of light sources, and amultiplexing unit configured to route the outputs of the plurality ofwavelength-specific multiplexers to the set of outputs. The controllermay be configured to simultaneously operate a first light source of thefirst set of light sources to generate light of a first wavelength and asecond light source of the second set of light sources to generate lightof a second wavelength separated from the first wavelength by less thana target separation amount. The multiplexing unit may configured tosimultaneously output light of the first wavelength and light of thesecond wavelength to at least one of the set of outputs.

In some of these variations, the target separation amount is 5nanometers. The multiplexing unit may include a cascaded network ofoptical couplers. Additionally or alternatively, the multiplexing unitmay include a first star coupler. In some of these variations, themultiplexing unit includes a second star coupler and a firstcontrollable switch optically coupled to a first wavelength-specificmultiplexer of the plurality of wavelength-specific multiplexers,wherein the first controllable switch may selectively route light to thefirst and second star couplers. In some variations, the light sourcemodule further comprises a wavelength locking unit. In some of thesevariations, each of the plurality of wavelength-specific multiplexers isoptically connected to a controllable switch, and the wavelength lockingunit is optically connected to the controllable switch.

In addition to the example aspects and embodiments described above,further aspects and embodiments will become apparent by reference to thedrawings and by study of the following description.

BRIEF DESCRIPTION OF THE DRAWINGS

FIG. 1 shows a side view of one example of an optical measurement systemas described herein.

FIGS. 2A and 2B illustrate schematic diagrams of example light sourcemodules that utilize a set of optical couplers to combine lightgenerated by corresponding light source sets.

FIG. 3 illustrates a schematic diagram of an example light source modulethat utilizes a set of multiplexers to combine light generated bycorresponding light source sets.

FIG. 4 depicts a variation of a controllable switch that may be usedwith the light source modules described herein.

FIGS. 5-9 show schematic diagrams of example light source modules thateach utilize a set of wavelength-selective multiplexers and amultiplexing unit to combine light generated by multiple light sourcesets.

FIG. 10 depicts a method of performing a spectroscopic measurement asdiscussed herein.

The use of the same or similar reference numerals in different figuresindicates similar, related, or identical items.

Additionally, it should be understood that the proportions anddimensions (either relative or absolute) of the various features andelements (and collections and groupings thereof) and the boundaries,separations, and positional relationships presented between them, areprovided in the accompanying figures merely to facilitate anunderstanding of the various embodiments described herein and,accordingly, may not necessarily be presented or illustrated to scale,and are not intended to indicate any preference or requirement for anillustrated embodiment to the exclusion of embodiments described withreference thereto.

DETAILED DESCRIPTION

Reference will now be made in detail to representative embodimentsillustrated in the accompanying drawings. It should be understood thatthe following description is not intended to limit the embodiments toany single embodiment. To the contrary, it is intended to coveralternatives, modifications, and equivalents as can be included withinthe spirit and scope of the described embodiments as defined by theappended claims. Likewise, although multiple embodiments are describedwith certain terminology, elements, and structures, it should beappreciated that any embodiment disclosed herein may incorporateterminology, elements, and/or structures disclosed with respect to otherembodiments.

The following disclosure relates to embodiments of optical measurementsystems, light source modules that may be used with these opticalmeasurement systems, and methods of performing measurements using theseoptical measurement systems. The optical measurement system may performa spectroscopic measurement using light (e.g., coherent or semi-coherentlight) of a plurality of different wavelengths, in which the opticalmeasurement system generates and emits the light from the opticalmeasurement system, and measures light received by the opticalmeasurement system. The light measured by the optical measurement systemmay be analyzed to determine one or more properties of the environmentsurrounding the optical measurement system (e.g., the presence, type,and/or one or more characteristics of an object measured by the opticalmeasurement system), collectively referred to herein as “spectroscopicinformation”.

As used herein, a “sample” refers to any object or substance positionedto receive light emitted from the optical measurement system and returnat least a portion of the light to the optical measurement system. Whenan optical measurement system as described herein is used to perform aspectroscopic measurement of a sample, coherent noise may limit theaccuracy of the spectroscopic measurement. Accordingly, the opticalmeasurement systems described herein may be configured to reducecoherent noise in spectroscopic measurements of a sample. As usedherein, “coherent noise” is an optical noise resulting from coherentinterference within a sample and that interferes with spectroscopicinformation being measured by the optical measurement system.

To help mitigate coherent noise, the optical measurement systemsdescribed herein may be configured to generate one or more groups ofwavelengths, and may simultaneously emit light at a given group ofwavelengths. The wavelengths within a given group may be selected to benearly identical, but separated by a certain amount. If the wavelengthsof a given group are properly spaced, they may be treated as a singlewavelength for the purpose of determining spectroscopic information in aspectroscopic measurement, yet also reduces the coherent noise for thespectroscopic measurement.

Also described herein are light source modules that include lightsources configured to generate these one or more groups of wavelengths.The light source modules may be configured to route light from theselight sources to one or more outputs. Each output may provide lightgenerated from the light source module to a corresponding launch site ofthe optical measurement system. Light may be emitted from the opticalmeasurement system from one or more launch sites, and each launch siteprovides a unique entry position and/or angle to a sample.

When the optical measurement systems described herein are used toperform a spectroscopic measurement, the optical measurement systemilluminates the sample with different wavelengths of light within atarget spectrum and measures the sample's response to these wavelengths.Depending on the application, an optical measurement system does notnecessarily need to measure the sample's response (e.g., the measuredspectroscopic information) to the entire target spectrum but instead maymeasure spectroscopic information using a discrete number or set ofwavelengths within the target spectrum. This may simplify the design ofthe optical measurement system by allowing it to incorporate individuallight sources that provide light outputs at these discrete wavelengths,rather than utilizing light sources providing light outputs across allwavelengths of the target spectrum.

Accordingly, in some embodiments, the optical measurement systemsinclude a plurality of light sources that can be utilized to emit lightat different wavelengths to reduce coherent noise. The opticalmeasurement systems may employ coherent light sources, such as lasers,that output light (e.g., provide “light output”) having relativelynarrow wavelength ranges. A given light source may be single-frequency(fixed wavelength) or may be tunable to selectively generate one ofmultiple wavelengths (i.e., the light source may be controlled to outputdifferent wavelengths at different times). A laser may include asemiconductor laser, such as a laser diode (e.g., a distributed Braggreflector laser, a distributed feedback laser, an external cavitylaser), a quantum cascade laser, or the like.

As used herein, a “bandwidth” refers to a range of wavelengths (which insome instances may be a single wavelength) associated with a givencomponent or operation. For example, the optical measurement system mayperform a spectroscopic measurement using a measurement bandwidth, whichrepresents the portion of the spectrum (i.e., the target spectrum) thatencompasses the plurality of wavelengths used to perform thespectroscopic measurement. Similarly, light emitted by a light sourcemay have a bandwidth, which represents the wavelength or wavelengths ofthe emitted light. When a value of a wavelength (or wavelengths) isdiscussed herein, this value may be a time-averaged wavelength value, oran instantaneous wavelength value. Additionally, while the term“bandwidth” is used herein to describe wavelengths, it should beunderstood that the principles discussed herein apply equally toembodiments where “bandwidth” refers to frequencies, insofar as anequivalent frequency exists for any given wavelength.

The coherent noise associated with a measurement is dependent on thewavelength of light used to perform that measurement. If twomeasurements are performed using different wavelengths, the coherentnoise from each measurement (also referred to herein as a “coherentnoise view”) may be correlated with each other by an amount that dependson how close the wavelengths are to each other. If two wavelengths aresufficiently close to each other, measurements performed using thesewavelengths will effectively have the same coherent noise. Conversely,if wavelengths are sufficiently separated, measurements performed usingthese wavelengths can be treated as having different coherent noisesources.

As used herein, the “coherent noise bandwidth” for a target wavelengthrefers to a range of wavelengths around the target wavelength for whichotherwise identical measurements taken at different wavelengths resultin highly correlated coherent noise. In other words, if an opticalmeasurement system were configured to take a first measurement whileemitting light at a first wavelength in a coherent noise bandwidth, thento take a second measurement while emitting light at a second wavelengthin the coherent noise bandwidth, then the first and second measurementswould have highly correlated coherent noise. In these instances, thefirst wavelength would be considered to be within the coherent noisebandwidth of the second wavelength, and vice versa. Similarly, both thefirst and second wavelengths may both be within the coherent noisebandwidth of an additional wavelength (or wavelengths).

What qualifies as “highly correlated” is largely dependent on theaccuracy constraints for a given system design and intended samplecharacteristics, but for the purposes of this application, two signals(e.g., signals representing the coherent noise of a measurement,spectroscopic measurements of a sample) are highly correlated if theyhave a correlation coefficient r that is greater than 0.5. It should beappreciated however, that some systems may be designed with a morestringent correlation requirement (e.g., r greater than 0.7 or r greaterthan 0.8), and may apply different correlation requirements whencomparing different types of signals.

Depending on what spectroscopic information is being measured by theoptical measurement system, the signal-to-noise ratio (“SNR”) forindividual measurements at different wavelengths can be limited bydifferent noise sources, such as a fundamental noise source or acoherent noise source. When a measurement at a given wavelength islimited by fundamental noise, the SNR may be increased by increasing theamount of light introduced into the sample for this wavelength. When ameasurement at a given wavelength is limited by coherent noise, the SNRwill not be improved by increasing the amount of light introduced intothe sample at this wavelength. In these instances, an opticalmeasurement system would need to utilize other techniques to improve SNRat these wavelengths.

Accordingly, the optical measurement systems described herein may beconfigured to emit light at multiple wavelengths that are treated as asingle wavelength for the purpose of calculating spectroscopicinformation. Depending on the design of the optical measurement system,as well as the sample and spectroscopic information being measured, theoptical measurement system can tolerate some wavelength deviations froma given target wavelength of the plurality of wavelengths and stillobtain a spectroscopic measurement that is effectively the same as if itwere taken using the target wavelength. Two or more wavelengths are“spectroscopically equivalent” for a given sample if otherwise identicalmeasurements taken at these wavelengths have highly correlated signalvalues. In some embodiments, measurements taken at spectroscopicallyequivalent wavelengths may be averaged together and any coherent noisemay become a zero mean; that is, the signals may converge and so resultin an averaged measured signal with less coherent noise.

For a given sample, there may be a range of wavelengths around a targetwavelength that are spectroscopically equivalent (referred to herein asthe “spectroscopic information bandwidth”), where the range is widerthan the coherent noise bandwidth for the target wavelength. The opticalmeasurement systems may be configured to take a measurement using agroup of wavelengths that are spectroscopically equivalent, but producedifferent coherent noise views. Specifically, two wavelengths producedifferent coherent noise views if one of the wavelengths is positionedoutside the coherent noise bandwidth of the other wavelength. In otherwords, the wavelengths are separated by an interstitial wavelength rangethat allows for the generation of different coherent noise views whilestill allowing the optical measurement systems to use measured lightfrom these wavelengths interchangeably. Thus, two different wavelengthsof light may be used to measure properties of a sample; thesewavelengths may be spectroscopically equivalent but provide differentnoise (e.g., have different noise profiles). Information from thesewavelengths may be used to reduce coherent noise without meaningfullyimpacting or compromising spectroscopic measurements or the associatedspectroscopic information calculated therefrom.

In this manner, although the wavelengths of the light emitted by theoptical measurement system are different from one another, they areclose enough to be spectroscopically equivalent with respect to theoptical measurement system's measurement capabilities. Put another way,the same sample attribute may be measured with different wavelengths oflight.

Because the spectroscopic information bandwidths for various wavelengthsare dependent on the type of sample, the optical measurement systemsdescribed herein may be designed to take measurements of a particulartype or types of sample (a “target sample type”). Accordingly, theoverall range of wavelengths that are emitted by an optical measurementsystem (e.g., the measurement bandwidth), as well as the selection ofany individual wavelengths within this range, may be selected based onthe target sample type and the spectroscopic information that will bemeasured. Additionally, when a group of spectroscopically identicalwavelengths that provide different coherent noise views are treated bythe optical measurement system as a single target wavelength, theselection of wavelengths with each group may be based on the overalldesign of the optical measurement system as well as the target sampletype and spectroscopic information that will be measured.

For example, in some embodiments, the target sample type is human skin,and the optical measurement system may derive physiological informationabout a user using a spectroscopic measurement. Other embodiments maymeasure attributes (e.g., the presence or amount of a chemical compoundor other component) of different target sample types, which may includegas (e.g., for environmental sensing), food (e.g., for determiningnutritional content), other objects, or the like. Where the sample ishuman skin, the spectroscopic information bandwidth (which may depend onthe wavelength of emitted light) may be on the order of three to fournanometers for many target wavelengths (such as certain wavelengths inthe infrared spectrum). At these target wavelengths, the coherent noisebandwidth may be on the order of a nanometer or less. Accordingly, insome instances where an optical measurement system is configured tomeasure skin, a group of wavelengths may be selected so that they arewithin four nanometers of each other (and thus may be spectroscopicallyequivalent), yet are separated by an interstitial range of at least onenanometer to thereby provide different coherent noise views.

Because the coherent noise bandwidth and the spectroscopic informationbandwidth may change with the composition of the sample and the designof the optical measurement system, different types of samples maynecessitate a different selection of wavelengths. In some instances,this may entail the use of different systems to measure different typesof samples. In other instances, an optical measurement system mayinclude enough light sources to generate the wavelengths necessary toperform measurements of multiple different target sample types. When theoptical measurement system is used to measure a first type of sample, afirst set of light sources may be selected and used to perform aspectroscopic measurement. When the optical measurement system is usedto measure a second type of sample, a different second set of lightsources may be selected and used to perform a spectroscopic measurement.

While changing the wavelength of the light emitted by the opticalmeasurement system may provide different coherent noise views, this isjust one way in which the optical measurement systems described here maymitigate coherent noise. For example, the coherent noise experienced bylight in a spectroscopic measurement may vary based on the path thelight takes through the sample, and thus may vary with a number offactors, such as the angle at which light enters the sample, scatteringproperties of the sample, the width of the light output, physicalgeometry of illumination and collection elements in an opticalmeasurement system, and so forth. As a result, the optical measurementsystems may be configured to measure light that has passed through awider volume of the sample, which may provide a range of differentcoherent noise views. Changing the wavelength of the light as discussedabove may be used to provide a different coherent noise view for a givenregion of the sample. This may also allow coherent noise to be reducedwithout exacerbating other noise sources in the optical measurementsystem, such as detector noise and laser noise.

Generally, the optical measurement systems and methods described hereinutilize a light source module to generate light used for spectroscopicmeasurements. Specifically, the light source modules described hereininclude multiple light sources that are integrated into a single module.In some instances, the light source module may be part of a photonicintegrated circuit. Light generated by the light source module may belaunched from the light source module or another portion of a photonicintegrated circuit incorporating the light source module at one or morelocations (e.g., via an outcoupler such as an edge coupler, a verticaloutput coupler, or the like). Light launched from the light sourcemodule may exit the optical measurement system (and any deviceincorporating the optical measurement system) at one or more launchsites toward a sample.

When an optical measurement system produces light at a group ofwavelengths that provide different coherent noise views but arespectroscopically equivalent, a light source module of the opticalmeasurement system may include two or more light sources, each of whichis configured to generate light at a corresponding wavelength of thegroup. These light sources may be run simultaneously, which effectivelydoubles the output power of the optical measurement system at a givenwavelength in instances when the optical measurement system treats thegroup of wavelengths as a single wavelength for the purpose ofcalculating spectroscopic information. In other instances, only one ofthese light sources is run at a time. For example, this may provideredundancy to the optical measurement system in case one of the twolight sources fails to operate as intended.

When the light source module is part of a photonic integrated circuit,the photonic integrated circuit may incorporate multiple components(e.g., a light source module, optical junction(s), and one or moremultiplexers) in a single package. In one sample embodiment, lightoutputs from the light sources may be tuned by an optical junction (suchas an interferometer or optical coupler as discussed below) which, inturn, transmits the light outputs to the multiplexer. The multiplexeroutputs a single light output having a bandwidth that is less than abandwidth of coherent noise from a sample, and in some instances can doso with approximately zero optical loss. As used herein, “zero opticalloss” may be understood to be a condition in which no loss is associatedwith the operation of the light source module, or less thanapproximately two to three percent optical loss is associated withoperation of the light source module. The light source module mayinclude components that are wavelength dependent (where there is awavelength dependency on transmission between an input or inputs and anoutput or outputs of the component) or wavelength independent (wherelight is transmitted between input(s) and output(s) of the componentregardless of its wavelength) for the wavelengths of light produced bythe light source module.

These and other embodiments are discussed below with reference to FIGS.1-10 . However, those skilled in the art will readily appreciate thatthe detailed description given herein with respect to these figures isfor explanatory purposes only and should not be construed as limiting.

As used throughout this specification, a reference number without analpha character following the reference number can refer to one or moreof the corresponding references, the group of all references, or some ofthe references. For example, “207” can refer to any one of the lightsources 207 (e.g., light source 207A1, light source 207B1, etc.), canrefer to all of the light sources 207, or can refer to some of the lightsources (e.g., both light source 207A2 and light source 207A1 in a lightsource set 210A) depending on the context in which it is used.

Representative applications of methods and apparatuses according to thepresent disclosure are described in this section. These examples arebeing provided solely to add context and aid in the understanding of thedescribed examples. It will thus be apparent to one skilled in the artthat the described examples may be practiced without some or all of thespecific details. Other applications are possible, such that thefollowing examples should not be taken as limiting.

FIG. 1 illustrates an optical measurement system 100, which may includean interface 180, a set of light sources 107, a detector 130, acontroller 140, an outcoupler 150, a diffuser 135, a lens 190, and asubstrate or photonics die 115. The set of light sources 107, outcoupler150, and associated photonics elements (such as those discussed belowwith respect to FIGS. 2A-9 , including optical couplers, multiplexers,and the like) are typically formed on or in the photonics die 115 toform a photonic integrated circuit. The photonic integrated circuit maybe part of a larger optical system that forms the optical measurementsystem.

The interface 180 can include an external surface of a device thatincorporates the optical measurement system 100 (and may form a portionof a housing of such a device). The interface 180 can accommodate lighttransmission therethrough, thereby allowing the optical measurementsystem to emit externally to a sample and receive light returnedtherefrom. The interface 180 includes at least one window that definesone or more emission regions (through which light emitted by the opticalmeasurement system 100 may exit the device) and one or more collectionregions (through which light entering the device may reach apredetermined portion of the optical measurement system 100, such asdetector 130).

In some examples, the optical measurement system 100 can include anaperture structure 160 including one or more regions (e.g., atransparent region 170, an opaque region, a translucent region, areflective region, a region having a different refractive index thansurrounding material, and so on) that define the emission and/orcollection regions of the interface 180. The aperture structure 160 maydirect and/or control the launch position (or positions) of the lightinto the sample 120 being measured by the optical measurement system100. By controlling the location and/or angles of light entering thesample 120, the light incident on the sample 120, and/or exiting fromthe sample 120, can be selectively configured. Although depicted in FIG.1 , the sample 120 is not included in the optical measurement system100.

While operating the optical measurement system 100, the sample 120 canbe located close to, or touching at least a portion of, the opticalmeasurement system 100, such as the interface 180. The set of lightsources 107 can be coupled to the controller 140, which may include oneor more processing units and control operation of each light source ofthe set of light sources 107. For example, the controller 140 can send asignal (e.g., current or voltage waveform) to control a given lightsource 107, which can thereby generate light. As mentioned above, theset of light sources 107 may collectively be able to generate light of aplurality of different wavelengths, which may be directed to the sample120 via the interface 180. Different wavelengths may be emittedsequentially, allowing a series of individual measurements to beperformed at different wavelengths. These individual measurements may beperformed with different durations depending on the wavelength. Theseindividual measurements may collectively form a spectroscopicmeasurement as described herein.

As mentioned above, the set of light sources 107 may include one or moregroups of light sources, where each group of light sources generateslight at a corresponding group of wavelengths that are spectroscopicallyequivalent but provide different noise views. In instances where aspectroscopic measurement includes a series of individual measurementstaken using different wavelengths, multiple light sources of one ofthese groups of light sources may be operated simultaneously during anindividual measurement, and the optical measurement system 100 mayconsider this individual measurement to have been performed at a singlewavelength for the purpose of calculating spectroscopic information.

Generally, the photonic integrated circuit may be configured such thatlight generated by each light source used in a given spectroscopicmeasurement can exit the optical measurement system from the samelocation (or set of locations). In this way, the individual measurementsperformed at different wavelengths may be introduced to a common portionof the sample 120. Accordingly, in some instances the light outputs fromthe light sources 107 may be combined into a single combined lightoutput or a set of combined light outputs from the photonics die 115(even if only a single wavelength may be emitted at a given time). Eachcombined light output may be collimated, focused, diffused, or otherwiseacted upon by optical elements such as the lens 190 before it reachesthe sample 120. Similarly, light returned from the sample may becollimated, focused, diffused, or otherwise acted upon by opticalelements before reaching the detector 130.

In instances where multiple light sources are generating lightsimultaneously, the combined light output may contain the light outputgenerated by each of these light sources 107, and the wavelengths ofthose light outputs generally remain unchanged. Certain embodiments mayuse or incorporate light sources 107 that output infrared light.“Infrared,” as used herein, refers to wavelengths of light that arelonger than visible light and generally have wavelength greater than 800nanometers. The light sources 107 in these instances may be configuredto emit any suitable infrared wavelengths, such as wavelengths in theshort-wavelength infrared spectrum and/or the mid-wavelength infraredspectrum. As discussed above, the range of wavelengths that may bespectroscopically useful for a given measurement may depend at least inpart on the type of sample 120 as well as the spectroscopic informationbeing measured.

Discussions herein may reference an optical measurement system 100, alight source module, a photonics die(s) 115, and/or a photonicintegrated circuit as emitting light, though this light actually mayinitially be generated by one or more of the light sources 107. As such,discussions of a given component emitting light is considered toencompass the underlying light source or sources that are generating thelight, so long as that light source or light source set is part of thatcomponent.

In some examples, the set of light sources 107 may generate light thatis manipulated by one or more elements within the photonics die 115 andultimately exits the photonics die 115 via an outcoupler 150. When thephotonics die 115 emits light in this manner, the light may be modifiedby one or more optical components before reaching the sample 120, asdiscussed above. For example, in the variation shown in FIG. 1 thislight output may be received by a lens 190. The lens 190 may be a freespace lens or include other free space optics; in some examples, thelens 190 instead may be multiple lenses that cooperate or coordinate tofocus a light output from the outcoupler 150. Additionally, the lens 190may perform multiple functions, such as collimating light, beamsteering, and/or beam shaping a light output from the photonics die 115.

In the embodiment shown in FIG. 1 , the light output from the lens 190may be directed to a diffusing element 135. The diffusing element 135may move in one or multiple dimensions and the movement of the diffusingelement 135 may be discrete or continuous. The diffusing element 135 maygenerate an illumination profile of light that is based at leastpartially on the angle spacing of light received from the lens 190 andthe total range of angles of light incident on the diffuser.

Depending on the nature of the measured sample 120, light can penetrateinto the sample 120 to reach one or more scattering sites and can return(e.g., reflect and/or scatter back) towards the optical measurementsystem 100. Depending on the design of the optical measurement system100 and the nature of the sample 120, light may travel within the sample120 according to a controlled path length distribution (i.e., a range ofpath lengths that a certain wavelength of light emitted from the opticalmeasurement system is expected to travel before returning to the opticalmeasurement system 100). The return light that enters back into theoptical measurement system 100 may be directed, collimated, focused,and/or magnified. The return light can be directed towards the detector130. The detector 130 can detect the return light and can send anelectrical signal indicative of the amount of detected light to thecontroller 140. This measured signal contains, and may be used with,measured signals from other measurements to calculate spectroscopicinformation related to the properties of the sample 120.

In some instances, some of the light emitted by the photonics die 115(and generated by one or more light sources 107) can optionally bedirected towards a reference (not illustrated in FIG. 1 ). The referencecan redirect light towards optics which may include, but are not limitedto, a mirror, lens, and/or a filter, and may direct, collimate, focus,and/or magnify light towards the detector 130. The detector 130 canmeasure light reflected from the reference and can generate anelectrical signal indicative of this reflected light for calibration ofthe optical measurement system 100 or other quality purposes.

The controller 140 can be configured to receive one or more electricalsignals from the detector 130; these electrical signals may be used(e.g., by controller 140 or another processor) to calculatespectroscopic information about the sample 120. For example, thedetector 130 may be configured to transmit the electrical signals to thecontroller 140, which calculates spectroscopic information therefrom. Insome instances, the detector may include a detector array with multiplesensing elements (e.g., an array of photodiodes), and the detector 130may output a different electrical signal for each sensing element. Eachsensing element of the detector array may collect light from a differentlocation or region of the sample 120, or, in instances where the opticalmeasurement system 100 includes a reference, light returned from thereference. In some instances, a given sensing element of the detector130 may receive light from different locations at different times andmay output a time-multiplexed signal corresponding to these locations.For example, a sensing element may alternate between measuring lightreceived from the sample 120 and light received by a reference.

As mentioned above, embodiments of the optical measurement systemsdescribed herein may be incorporated into a device (e.g., which may havea housing that includes the interface 180). The device, which in someinstances is configured to be wearable by a user, may operate solely totake measurements using the optical measurement system or may be amulti-functional device capable of performing additional functions (notdiscussed in detail herein). For example, in some instances the opticalmeasurement system may be incorporated into a smart phone, tabletcomputing device, laptop or desktop computer, a smartwatch, or otherelectronic device (collectively referred to herein as “electronicdevices” for ease of discussion).

FIGS. 2A-9 show different embodiments of light source modules that maybe used to route light from a plurality of light sources to acorresponding set of outputs. The light source modules may beincorporated into a photonic integrated circuit (e.g., the photonicintegrated circuit including the light sources 107 and photonics die 115of the optical measurement system 100 of FIG. 1 ), and light received atthese outputs may be emitted from the photonic integrated circuit, suchas via an outcoupler. Accordingly, light from each output of lightsource module may be used to provide light to one or more launch sitesof the optical measurement system.

FIG. 2A illustrates an example light source module 200. The light sourcemodule 200 may include multiple light source sets 210 of light sources207, a set of optical couplers 225, and a set of multiplexers 235. Asshown there, each light source set 210 is optically connected to (i.e.,coupled in manner that allows light transmission to) each of the set ofmultiplexers 235 via an optical coupler 225, such that each multiplexer235 receives a portion of the light generated by each light source 207.As a result, each multiplexer 235 is optically connected to every lightsource 207, and may output light it receives from any of the lightsources 207 that are active at a given time. The output of themultiplexers 235 may form the outputs of the light source module 200.

Individual elements of a group depicted in FIG. 2A, such as the lightsources 207, may be referred to with a separate element number 207A1,207A2, 207B1, 207B2, and so forth. For example, FIG. 2A depicts threelight source sets 210 (a first light source set 210A, a second lightsource set 210B, and a third light source set 210N), each of whichincluding two light sources 207 (the first light source set 210A hasfirst and second light sources 207A1, 207A2, the second light source set210B has first and second light sources 207B1, 207B2, and the thirdlight source set 210N has first and second light sources 207N1, 207N2).The set of optical couplers 225 is shown as having three opticalcouplers 225 (first optical coupler 225A, second optical coupler 225B,and third optical coupler 225N). Finally, the set of multiplexers 235includes a first multiplexer 235A and a second multiplexer 235B. Theoperation of the light source module 200 is described using the firstlight source set 210A and the first optical coupler 225A, though itshould be appreciated that these principles may be applied to the otherlight source sets 210 and their corresponding optical couplers 225.Indeed, the light source module 200 may include any suitable number oflight source sets 210 and corresponding optical couplers 225 as may bedesired.

Generally, the light sources 207 of a given light source set 210 may beconfigured to generate light at wavelengths that are close to eachother. For example, the light sources 207A1 and 207A2 of the first lightsource set 210A may emit light of the same wavelength or differentwavelengths of light. In some examples, the light sources 207 emit thesame wavelength of light. Because the light sources 207A1 and 207A2 areindependently controllable and may be used individually or may be usedat the same time, the light source module 200 may provide redundancy forthe optical measurement system.

Some light sources may fall outside the specifications or may not befunctioning as designed; in this case, redundancy of light sources mayat least partially resolve these issues. For example, as long as one ofthe light sources 207A1 and 207A2 of the first light source set 210A isproperly functioning, the first light source set 210A may still providelight to both multiplexers 235. In the event that one of the lightsources, such as light source 207A1 should fail, then light source 207A2may be used and vice versa. Conversely, if each of the light sources207A1 and 207A2 are optically connected to a single multiplexer (e.g.,light source 207A1 is optically connected only to the first multiplexer235A and light source 207A2 is optically connected only to the secondmultiplexer 235B), failure of one of these light sources would result inthe corresponding multiplexer 235 being unable to receive any light ofthat wavelength.

When the light sources 207A1 and 207A2 simultaneously emit light, thismay allow for increased output power at each of the multiplexer 235outputs. If the light sources 207A1 and 207A2 are capable of producingapproximately the same optical power, generating light from both lightsources simultaneously thus allows the output power of the light sourcemodule 200 to be approximately doubled for that wavelength (as comparedto when only one of the light sources 207A1 and 207A2 is used). Thus,the light source module 200 may provide redundancy and/or increasedpower output per wavelength of light for any light source sets 210 thatgenerate the same wavelength of light. Additionally, the light sources207A1 and 207A2 may emit the same wavelength of light at approximatelythe same intensity, but need not (e.g., one light source 207 from alight source set 210 may be configured and/or controlled to generate adifferent intensity of light as compared to that of other light sourceswithin that light source set 210).

In some examples, the light sources 207 from a light source set may beconfigured to generate light at different wavelengths. In somevariations the light sources 207A1 and 207A2 of the first light sourceset 210A may emit light at wavelengths that are spectroscopicallyequivalent and/or produce different coherent noise views forspectroscopic measurements of a target sample type performed by anoptical measurement system that incorporates the light source module200. In some variations, the wavelengths generated by light sources207A1 and 207A2 of the first light source set are separated by less thanfour nanometers (e.g., the wavelength of light generated by the lightsource 207A1 is less than four nanometers apart from the wavelength of alight output by the light source 207A2). In some of these variations,the wavelengths generated by light sources 207A1 and 207A2 of the firstlight source set are separated by less than four nanometer. This limitedwavelength separation may cause the first light source set 210A toproduce spectroscopically equivalent wavelengths for a givenspectroscopic measurement performed by an optical measurement system asdiscussed previously.

Because the optical measurement system may treat light measured at thesedifferent wavelengths as a single wavelength for the purpose ofcalculating spectroscopic information, the light sources 207A1 and 207A2may be operated independently to provide the redundancy and increasedoptical power described immediately above. Accordingly, as long as oneof the light sources 207A1 and 207A2 of the first light source set 210Ais properly functioning, the first light source set 210A may stillprovide light to both multiplexers 235 that may be usable by an opticalmeasurement system to perform a spectroscopic measurement.

Additionally or alternatively, the wavelengths generated by lightsources 207A1 and 207A2 of the first light source set 210A are separatedby at least one nanometer (e.g., the wavelength of light generated bythe light source 207A1 is at least one nanometer apart from thewavelength of a light output by the light source 207A2). For certainspectroscopic measurements performed by an optical measurement system,this wavelength separation may provide different coherent noise viewsfrom each light source 207 within a given light source set 210. Thiscoherent noise may be averaged out to reduce the noise associated withthe spectroscopic measurements.

In some instances, each light source set 210 is configured to produce adifferent wavelength or wavelengths. Indeed, while the light sourceswithin a given light source set 210 may generate a single wavelength ormultiple closely-spaced wavelengths as discussed above, the wavelengthor wavelengths generated by one light source set may be separated fromthe wavelength or wavelengths generated by another light source set by arelatively large amount (e.g., spanning tens or hundreds of nanometers).For example, in some instances, any wavelength (or wavelengths)generated by the first light source set 210A is not spectroscopicallyequivalent to any wavelength (or wavelengths) generated by the secondlight source set 210B. This may allow the light source sets 210 tocollectively emit light across a broad spectrum of wavelengths, whichmay thereby facilitate spectroscopic measurements using this broadspectrum of wavelengths.

As mentioned above, each light source set 210 is optically connected toa corresponding optical coupler 225. Each coupler 225 has two inputs andtwo outputs, where each input is optically connected to a correspondinglight source 207 of the light source set 210 and each output isconnected to a corresponding multiplexer 235 of the set of multiplexers.The optical coupler 225 splits a portion of the light received at eachinput between the outputs, thereby routing light generated from eachlight source 207 of a light source set 210 to both the first multiplexer235A and the second multiplexer 235B.

For example, the first optical coupler 225A may receive light from thelight source 207A1 on a first input of the first optical coupler 225Aand may receive light from the light source 207A2 on a second input ofthe first optical coupler 225A. Similarly, the second optical coupler225B may receive light from the second light source set 210B at itsinputs and the third optical coupler 225N may receive light from thethird light source set 210N. Similarly, each of the first, second, andthird optical couplers 225A, 225B, and 225N may provide light to themultiplexers 235A and 235B. For example, a first output of the firstoptical coupler 225A is optically connected to the first multiplexer235A and a second output of the second optical coupler 225 is connectedto the second multiplexer 235B. The optical connections between thelight sources 207 and the optical couplers 225, and between the opticalcouplers 225 and the multiplexers 235 are illustrated in FIG. 2A aslight paths 245. In some examples, such as when the light source module200 is incorporated into a photonic integrated circuit, the light paths245 are waveguides.

Each optical coupler 225 may be any suitable optical coupler, such as awavelength independent directional coupler, having two inputs and twooutputs. Example optical couplers 225 include a Mach-Zehnderinterferometer (MZI), or a multimode interferometer (MMI) (e.g., a 2×2MMI), or the like. When light is received by an optical coupler 225 atan input thereof, the optical coupler 225 is configured to split thislight between the outputs according to a predetermined splitting ratio.For example, each optical coupler 225 may be configured such thatoptical power received from each light source 207 (i.e., at acorresponding input of the optical coupler 225A) may be split toapproximately equally each of the outputs. In these instances, when thelight sources 207A1 and 207A2 of the first light source set 210simultaneously generate light, the first output of the first opticalcoupler 225A (and thus the first multiplexer 235A) will receive half ofthe light generated by light source 207A1 and half of the lightgenerated by light source 207A2. Similarly, the second output of thefirst optical coupler 225A (and thus the second multiplexer 235B) willreceive the other half of the light generated by light source 207A1 andthe other half of the light generated by light source 207A2.

In some instances, the set of optical couplers 225 may be replaced witha set of 2×2 controllable switches. An example controllable switch isdescribed below with respect to FIG. 4 , and may be controlled toselectively route light from either light source 207 of a light sourceset 210 to one or both of the set of multiplexers 235. Specifically, afirst input of a controllable switch is optically connected to one lightsource 207 of a light source set 210 and the second input of thecontrollable switch is optically connected to the other light source 207of the light source set 210. Similarly, a first output of thecontrollable switch is optically connected to the first multiplexer 235Aand a second output of the controllable switch is connected to thesecond multiplexer 235B. In these instances, the controllable switch maybe controlled to adjust how light received at a given light source issplit between the multiplexer 235.

Each multiplexer 235 of the set of multiplexers 235 may be anymultiplexer capable of combining multiple inputs corresponding to themultiple wavelengths received from the various light source sets into aset of outputs (though it should be appreciated that a multiplexer 235may only receive light at a single input at a given point in time). Insome examples, the multiplexers 235 may be wavelength-selectivemultiplexers such as an Echelle grating multiplexer, an arrayedwaveguide grating (AWG) multiplexer, a ring resonator multiplexer, orthe like. In instances where the couplers 225 are configured to equallysplit light between their outputs, each multiplexer 235 receives halfthe light generated by a given light source set 210. Accordingly, eachmultiplexer 235 can output half the light generated by that light sourceset 210 to be used elsewhere in the system. For example, an opticalmeasurement system may output light to multiple regions of a sample(e.g., via different launch sites of the optical measurement system),and the first multiplexer 235A may output light to a first launch site(or set of launch sites) and the second multiplexer 235B may outputlight to a second site (or set of launch sites). In some instances, theoutput of a multiplexer 235 is split to provide additional outputs ofthe light source module 200.

The multiplexers 235 may be able to multiplex multiple differentwavelengths of light from a given light source set with minimal opticallosses. In some examples, the wavelength bandwidth of the multiplexer235 (i.e., the range of wavelengths that may pass through a given inputchannel and still be routed to the output channel) may be less thanapproximately five to ten nanometers depending on the design of themultiplexer 235. Accordingly, if the wavelengths produced by a lightsource set are sufficiently close (such as the wavelengths separated byless than four nanometers discussed above) these different wavelengthsmay be introduced to the same input channel of the multiplexer 235 andbe multiplexed with little optical loss. Conversely, it may be difficultto add a separate channel to a multiplexer 235 for each of thesewavelengths without increasing the optical losses.

While two multiplexers 235 are shown in FIG. 2A, it should beappreciated that in some instances the light source module 200 includesmore than two multiplexers 235. In these embodiments, the light sourcemodule 200 may include multiple optical couplers that optically connecta light source set 210 to the set of multiplexers. For example, in someinstances, each output of the optical couplers 225 shown in FIG. 2A maybe optically connected to a corresponding 1×2 optical coupler (notshown). Each output of the 1×2 couplers is optically connected to arespective multiplexer 235, thereby optically connecting a light sourceset 210 to four multiplexers. Similarly, a light source set may includemore than two light sources 207 (e.g., three or four light sources), andadditional optical couplers may be used to combine the light generatedfrom these light sources and route them to the multiplexers 235.

The light sources within a given light source set 210 (e.g., the lightsources 207A1 and 207A2 of the first light source set 210) may be formedon the same substrate or may be formed on different substrates. Ininstances where the light sources 207 of a light source set 210 areformed on the same substrate, they may be positioned immediatelyadjacent to each other (i.e., with no intervening light sources 207) ormay be positioned with one or more light sources 207 (e.g., from adifferent light source set) positioned therebetween.

As shown in FIG. 2A, the waveguides may cross one another in between theoptical couplers 225 and the multiplexers 235, though in othervariations the light source module may be configured so that thewaveguides do not cross. FIG. 2B illustrates an example light sourcemodule 250. The light source module 250 is similar to the light sourcemodule 200 of FIG. 2A and includes multiple light source sets 210 oflight sources 207, optical couplers 225, and multiplexers 235 discussedpreviously, except that the light paths 255 connecting the opticalcouplers 225 and the multiplexers 235 are routed so that they do notcross each other. Because the light paths do not cross each other, lesslight may couple between the waveguides due to the lack of proximity toone another.

FIG. 3 illustrates an example light source module. The light sourcemodule 300 of FIG. 3 includes light source sets 310, light sources 307,a set of multiplexers 315, and multiplexer 335. In some examples anddistinct from FIGS. 2A and 2B, the multiplexers 315 may be wavelengthdependent and the light source module 300 supplies one output of light.The single light output of the multiplexer 335 may allow the lightsource module 300 to be smaller in physical size than the lightsplitting systems such as the light source modules 200 and 250 discussedwith respect to FIGS. 2A and 2B, respectively. The output of themultiplexer 335 may still be split to allow the light source module 300to provide multiple outputs to be used by the optical measurementsystem.

Similar to the discussion of FIGS. 2A and 2B, in FIG. 3 , the lightsources 307 may provide light to the set of multiplexers 315, which maythen provide light to the multiplexer 335. Specifically, each lightsource set 310 is associated with a corresponding multiplexer 315 of theset of multiplexers 315. A first light source 307 of a light source set310 is optically connected to a first input of a correspondingmultiplexer 315 and a second light source 307 of the light source set310 is optically connected to a second input of the correspondingmultiplexer 315. The multiplexer 315 combines the light from its inputsinto a common output, which is optically connected to a correspondinginput of the multiplexer 335. The multiplexer 335 may combine lightreceived by its inputs (though it should be appreciated that in someinstances the multiplexer 335 only receives light at one of its inputsat a given time) into a common output, which may be utilized the opticalmeasurement system to perform a spectroscopic measurement as discussedabove.

Because the multiplexers 315 are wavelength specific, they are used tocombine different wavelengths of light generated by the light source set310, such as when a given light source set 310 is used to generatewavelengths with different coherent noise views as discussed above. Forexample, the wavelengths generated by light sources 307A1 and 307A2 ofthe first light source set 310A are separated by at least one nanometer(e.g., the wavelength of light generated by the light source 307A1 is atleast one nanometer apart from the wavelength of a light generated bythe light source 307A2). Each of the light source sets may be similarlyconfigured. Additionally, the wavelengths of a given light source setmay be positioned close enough to each other to allow these wavelengthsto be multiplexed by multiplexer 335 without incurring significantlosses. The light sources 307 of a given light source set 310 may beoperated simultaneously or sequentially, and may be used to provideredundancy and/or increase optical power as discussed above.

The set of multiplexers 315 and multiplexer 335 may include any suitablemultiplexers such as those discussed above, and each of thesemultiplexers may be designed specifically for the wavelengths beingmultiplexed. For example, a first multiplexer 315A may be designed tomultiplex the wavelengths generated by the light sources 307A1 and 307A2of the first light source set 310A, while a second multiplexer 315B maybe designed to multiplex the wavelengths generated by the light sources307B1 and 307B2 of the second light source set 310B.

In some instances, the set of multiplexers 315 may be replaced with aset of 2×2 controllable switches, such as discussed above. Specifically,a first input of a controllable switch is optically connected to onelight source 307 of a light source set 310 and the second input of thecontrollable switch is optically connected to the other light source 307of the light source set 310. Similarly, a first output of thecontrollable switch is optically connected to the multiplexer 335 and asecond output of the controllable switch is left disconnected, such thateach 2×2 controllable switch acts as a 2×1 switch. In these instances,the controllable switch may be controlled whether light generated from afirst light source 307 of a light source set 310 or a second lightsource 307 of the light source set 310 is routed to the multiplexer 335.

For example, FIG. 4 depicts a variation of a controllable switchsuitable for use with the light source modules described herein. FIG. 4shows a variation of a 2×2 controllable switch 400 having two inputs (afirst input 402 and a second input 403) and two outputs (a first output404 and a second output 406). As shown there, the controllable switchhas a first 2×2 coupler 408, a 2×2 coupler 410, and a controllable phasetuner 412 positioned between the first 1×2 coupler 408 and the second2×2 coupler 410. In the variation of 2×2 controllable switch 400 shownin FIG. 4 , the first 2×2 coupler 408 uses the first input 402 andsecond input 403 as inputs, and uses a first leg 414 and a second leg416 as outputs. Light received by either the first input 402 or thesecond input 403 of the 2×2 controllable switch 400 is split by thefirst 2×2 coupler 408 between the first leg 414 and the second leg 416.

Similarly, the second 2×2 coupler 410 receives light from the first leg414 and the second leg 416 as inputs and uses the first output 404 andthe second output 406 of the 2×2 controllable switch 400 as outputs.Light received by each input of the second 2×2 coupler 410 is splitbetween the first output 404 and the second output 406 according to acorresponding predetermined splitting ratio. It should be appreciatedthat the first input 402, second input 403, first output 404, secondoutput 406, first leg 414, and second leg 416 may each be a waveguide.

The relative amounts of light that are coupled into the first output 404and the second output 406 depend at least on 1) relative amounts oflight in the first leg 414 and the second leg 416 as it enters thesecond 2×2 coupler 410, 2) the phase difference between the light in thefirst leg 414 and the second leg 416 as it enters the 2×2 coupler 410,and 3) the wavelength of the light. As such, changing the phasedifference between the first leg 414 and the second leg 416 changes thedistribution of light between the first output 404 and the second output406. By adjusting the phase difference between the first leg 414 and thesecond leg 416, the 2×2 controllable switch 400 may take light receivedfrom one of its inputs (e.g., the first input 402 or the second input403) and selectively route light entirely to the first output 404,entirely to the second output 406, or simultaneously to both the firstoutput 404 and the second output 406 (i.e., split between the outputsaccording to a target splitting ratio). Furthermore, control of thecontrollable phase tuner 412 may be adjusted to account for thewavelength of light introduced into the 1×2 controllable switch, suchthat a desired output of the 2×2 controllable switch may be achieved forany of the wavelengths used to perform a spectroscopic measurement.

To adjust the phase difference between the first leg 414 and the secondleg 416, the controllable phase tuner 412 includes one or more phaseshifters that selectively modulate the phase of light passing througheither the first leg 414 or the second leg 416. Examples of suitablephase shifters include, for example, electrooptic phase shifters thatchange the refractive index of a portion of a waveguide using an appliedelectric field (e.g., via carrier injection), thermo-optic phaseshifters that change the refractive index of a portion of a waveguide bychanging its temperature, and optomechanical phase shifters (e.g., aMEMS phase shifter) where a moveable structure (e.g., a suspendedwaveguide) is moved to change an amount evanescent coupling with thewaveguide.

The controllable phase tuner 412 may include a single phase shifterpositioned to change the phase of light in one leg (either the first leg414 or the second leg 416), or may include multiple phase shifters (eachof which may be independently controlled). In some instances, thecontrollable phase tuner 412 includes multiple phase shifters where atleast one phase shifter is positioned to change the phase of light inthe first leg 414 and at least one phase shifter is positioned to changethe phase of light in the second leg 416. Additionally or alternatively,the controllable phase tuner 412 may include multiple phase tunerspositioned to change the phase of light in one of the legs. In thevariation of the 2×2 controllable switch 400 shown in FIG. 4 , thecontrollable phase tuner 412 includes a single phase shifter 418positioned to change the phase of light in the first leg 414.

In some instances, a controllable switch may also be configured to tapoff a portion of light received by the controllable switch. This may bedesirable in an instance where a light source module is used to passlight to a wavelength locking unit as described below with respect toFIG. 9 . For example, the 2×2 controllable switch 400 shown in FIG. 4includes a tap 420 (e.g., an optical waveguide tap) that extracts aportion of the light from a leg of the controllable switch 400 into aseparate waveguide 422. The waveguide 422 may carry light to anotherportion of the optical measurement system (e.g., a wavelength lockingunit as discussed herein). While shown as tapping light from a leghaving a phase shifter (the first leg 414 in FIG. 4 ), the tap 420 mayalternatively tap light from a leg that does not include a phase shifter(the second leg 416 in FIG. 4 ).

In other instances, a controllable switch may be configured as a 1×2 or2×1 controllable switch. In some of these variations, a controllableswitch may include a 1×2 coupler instead of the first 2×2 coupler 408 orthe second 2×2 coupler 410, which would change the 2×2 controllableswitch 400 discussed above into a 1×2 controllable switch or a 2×1controllable switch, respectively. Alternatively, one input of the first2×2 coupler 408 may be left disconnected such that the other input ofthe 2×2 coupler acts as the single input of the 1×2 controllable switch.Similarly, one output of the second 2×2 coupler 410 may be leftdisconnected, such that the other output of the second 2×2 coupler 410acts a single output of the 2×1 controllable switch. In these instances,the second 2×2 coupler 410 may be configured with an imbalance topromote coupling light into the output of the 2×1 controllable switch.

When the variations of the light source modules described above withrespect to FIGS. 2A-3 , are used to combine the outputs of a lightsource set having similar wavelengths (e.g., pairs of light sourcesemitting light at wavelengths separated by less than a handful ofnanometers as discussed above), these outputs are combined before theyare multiplexed with the outputs of other light source sets.Accordingly, a single light path (e.g., waveguide) is used to transferany light generated by a given light source set to a corresponding inputof a wavelength-selective multiplexer such as the multiplexers 235A,235B, or 335 discussed previously. Because different wavelengths oflight are introduced into a single input of the wavelength-selectivemultiplexer, there may be some intrinsic loss associated with thismultiplexing. While this intrinsic loss may be relatively small in manyinstances, this loss may increase as spacing between wavelengths in alight source set increases, and may further increase if any of the lightsources are chirped during operation.

FIG. 5 shows another variation of a light source module 500 as describedherein. Specifically, the light source module 500 includes a pluralityof light sources 502, each of which is configured to generate light at acorresponding wavelength. These light sources 502 include one or morepairs of light sources 502, where the wavelengths of light sources areseparated by less than a target separation amount. In some instances,this target separation may be selected so that these light sources 502generate spectroscopically equivalent wavelengths. The target separationwill be discussed in this embodiment as 5 nanometers (i.e., each ofthese pairs of light sources 502 generate light at correspondingwavelengths separated by less than 5 nanometers), though it should beappreciated that other values may be selected based on the system (e.g.,4 nanometers or 3 nanometers as discussed above).

In some instances, the light source module 500 includes at least oneadditional light source 502 that is not part of a pair as discussedabove (referred to herein as an “unpaired light source”). For each suchunpaired light source 502, the wavelength of light generated by thatlight source 502 is separated by at least the target separation amount(e.g., 5 nanometers) from the wavelengths produced by the remaininglight sources 502 of the light source module 500. For example, FIG. 5shows a set of unpaired light sources 504 and a set of paired lightsources 506. The set of unpaired light sources 504 includes one or moreunpaired light sources (e.g., light sources 502A-1 to 502A-N) eachhaving a corresponding wavelength (e.g., λ_(A-1) to λ_(A-N)).

The set of paired light sources 506 includes a plurality of lightsources (e.g., light sources 502B-1 to 502B-M) that form one or morelight source pairs that generate wavelengths separated by less than thetarget separation. In the light source modules described in relation toFIGS. 2A, 2B, and 3 , the outputs of these light source pairs are firstcombined before they are combined with the outputs of other lightsources. Conversely, in light source module 500, each light source of agiven light source pair is divided into a different subset of lightsources 502. For example, as shown in FIG. 5 , the set of paired lightsources 506 includes a first light source subset 508 and a second lightsource subset 510. There are N different light source pairs shown inFIG. 5 (which may be the same or a different number as the number oflight sources in the set of unpaired light sources 504), and each lightsource pair includes one light source in the first light source subset508 and one light source in the second light source subset 510. Forexample, a first light source pair may include a first light source502B-1 that is part of the first light source subset 508 and a secondlight source 502B-N+1 that is part of the second light source subset510. The first light source 502B-1 has a wavelength λ_(B-1) and thesecond light source 502B-N+1 has a wavelength λ_(B-1)+Δ₁ (where Δ₁ isless than the target separation amount). Similarly, a second lightsource pair may include a first light source 502B-2 that is part of thefirst light source subset 508 and a second light source 502B-N+2 that ispart of the second light source subset 510, and generate wavelengthsthat are separated by a Δ₁ that is also less than the target separationamount. In some instances, the light sources 502 within a given lightsource subset (e.g., the first light source subset 508 and/or the secondlight source subset 510) may generate wavelengths that are all separatedby at least the target separation within the light source subset.

The light sources 502 of the set of unpaired light sources 506, thefirst light source subset 508 and the second light source subset 510 maybe multiplexed using a set of wavelength-specific multiplexers 512.Specifically, the set of unpaired light sources 506 is multiplexed usinga first wavelength-specific multiplexer 512A, such that an output ofeach of the light sources 502A-1 to 502A-N is optically connected (e.g.,via a waveguide) to a corresponding input of the first multiplexer 512A.The first light source subset 508 is multiplexed using a secondwavelength-specific multiplexer 512B, such that an output of each of thelight sources 502B-1 to 502B-N is optically connected (e.g., via awaveguide) to a corresponding input of the second multiplexer 512B.Similarly, the second light source subset 510 is multiplexed using athird wavelength-specific multiplexer 512C, such that an output of eachof the light sources 502B-N+1 to 502B-M is optically connected (e.g.,via a waveguide) to a corresponding input of the third multiplexer 512C.It should be appreciated that in some instances the second multiplexer512B and/or the third multiplexer 512C may also multiplex the outputs ofone or more unpaired light sources in addition to the set of pairedlight sources.

Each of the wavelength-specific multiplexers 512A, 512B, and 512C may betailored to specific wavelengths produced by light sources 502 connectedthereto. Because the pairs of light sources are divided between thelight source sets 508 and 510, they will each be multiplexed by adifferent wavelength-specific multiplexer, and thus each of the secondmultiplexer 512B and the third multiplexer 512C may be designed withadditional space between the inputs to these multiplexers as compared toinstances where the light sources of a given pair are opticallyconnected to different inputs of a single multiplexer.

The first wavelength-specific multiplexer 512A has an output 518A thatwill output light generated by each light source of the set of unpairedlight sources 504. The second wavelength-specific multiplexer 512B hasan output 518B that will output light generated by each light source ofthe first light source subset 508. The third wavelength-specificmultiplexer 512C has an output 518C that will output light generated byeach light source of the second light source subset 510. Each of theseoutputs 518A, 518B, and 518C may be optically connected to amultiplexing unit 514 that routes light from each of the outputs 518A,518B, and 518C to a common set of outputs for the light source module500.

Accordingly, light emitted by a given light source 502 will be routedthrough one of the wavelength-specific multiplexers 512A, 512B, or 512Cand the multiplexing unit 514 before it is outputted from the lightsource module 500. Each output of the common set of outputs may becapable of outputting light from every light source 502 of the set ofunpaired light sources 506, the first light source subset 508 and thesecond light source subset 510 (though it should be appreciated thatthat the multiplexing unit 514 may also include one or more additionaloutputs that are only capable of outputting light from a subset of theselight sources). This allows a wide range of wavelengths to be routed acommon output or outputs of the light source module 500. When used in anoptical measurement system as described herein, this allows light of anyof the wavelengths generated by the light source module 500 to belaunched from a given launch site to perform spectroscopic measurements.

When a spectroscopic measurement is performed by taking a plurality ofindividual measurements at different wavelengths, either one or twolight sources of the light source module 500 may be active at a giventime. For example, when an individual measurement is performed using awavelength associated with an unpaired light source, the correspondinglight source may be the only light source actively generating lightduring the individual measurement. Conversely, when an individualmeasurement is performed using a wavelength associated with a pairedlight source, either of both of the paired light sources may be activelygenerating light during a given individual measurement. As discussedabove, if the wavelengths generated by the light source pair arespectroscopically equivalent for a given spectroscopic measurement,generating light simultaneously with a light source pair may increase(e.g., double) the optical power for that measurement, as the opticalmeasurement system will treat this light as if it were generated at asingle wavelength for the purpose of calculating spectroscopicinformation. When the wavelengths are selected to provide differentcoherent noise views, this may also reduce coherent noise associatedwith the spectroscopic measurement. Alternatively, a single light sourceof a pair may be active at a time, for example in stances where theadditional optical power is not needed or when the other light source ofthe pair is not functioning properly. Accordingly, in some instances agiven spectroscopic measurement includes a plurality of individualmeasurements using different pairs of light sources, where both lightsources simultaneously generate light at different wavelengths, and mayfurther include one or more additional individual measurements duringwhich a single wavelength of light is generated (e.g., via a singlelight source).

The multiplexing unit 514 may include any component or componentscapable of routing the outputs of the set of multiplexers 512 to acommon set of outputs 516. Because each input to the multiplexing unit514 can include a range of wavelengths depending on which light source502 is active at a given moment, the multiplexing unit 514 may leveragewavelength-independent components to route light.

FIG. 6 shows one example of a light source module 600 utilizing amultiplexing unit 614 having a star coupler 622. As shown there, thelight source module 600 includes a set of unpaired light sources 604 anda set of paired light sources 606 divided into a first light sourcesubset 608 and a second light source subset 610. These light sources 602may be configured as discussed above with respect to the light sourcemodule 500 of FIG. 5 . For the sake of illustration, four light sources602A-1, 602A-2, 602A-N-1 and 602A-N (that generate correspondingwavelengths λ_(A-1), λ_(A-2), λ_(A-N-1), and λ_(A-N)) that represent aset of N light sources are shown in the set of unpaired light sources604. Similarly, four sets of paired light sources are shown in FIG. 6 .This includes a first pair of light sources 602B-1 and 602B-5 thatgenerate wavelengths separated by a first separation amount Δ₁, a secondpair of light sources 602B-2 and 602B-6 that generate wavelengthsseparated by a second separation amount Δ₂, a third pair of lightsources 602B-3 and 602B-7 that generate wavelengths separated by a thirdseparation amount Δ₃, and a fourth pair of light sources 602B-4 and602B-8 that generate wavelengths separated by a fourth separation amountΔ₄. Each of the separation amounts Δ₁- Δ₄ are less than a targetseparation amount as discussed. The first light source set 608 includesa first light source from each light source pair (e.g., 602B-1, 602B-2,602B-3, and 602B-4) and the second light source set 608 includes asecond light source from each light source pair (e.g., 602B-5, 602B-6,602B-7, and 602B-8).

The outputs of the light sources from the set of unpaired light sources604, the first light source subset 608, and the second light sourcesubset 610 are respectively multiplexed by a first wavelength-selectivemultiplexer 612A, a second wavelength-selective multiplexer 612B, and athird wavelength-selective multiplexer 612C as discussed above. Thefirst wavelength-specific multiplexer 612A has an output 618A that willoutput light generated by each light source of the set of unpaired lightsources 604. The second wavelength-specific multiplexer 612B has anoutput 618B that will output light generated by each light source of thefirst light source subset 608. The third wavelength-specific multiplexer612C has an output 618C that will output light generated by each lightsource of the second light source subset 610. Each of these outputs618A, 618B, and 618C may be optically connected to the multiplexing unit614.

As mentioned previously, the multiplexing unit 614 includes a starcoupler 622. In the variation shown in FIG. 6 , the star coupler 622 isconfigured as a 3×N star coupler with 3 inputs and N outputs 616. Inthese instances, the three outputs 618A, 618B, and 618C of the set ofmultiplexers 612A, 612B, and 612C act as the inputs to the star coupler622, while the N outputs 616 may act as outputs of the light sourcemodule 600. Accordingly, the N outputs 616 may be any suitable number ofoutputs 616 as may be desired. The star coupler 622 is wavelengthindependent such that light received at any input of the star coupler622 will be split between the N outputs 616 regardless of the wavelengthof light received at that input. Accordingly, light may be generated byany light source of the set of unpaired light sources 604 and the set ofpaired light sources 606, and that light will be split between the Noutputs 616 of the star coupler 622. The set of multiplexers 612A, 612B,and 612C, as well as the star coupler 622 may have little to nointrinsic optical loss, and may thereby provide a low-loss way to couplelight from a set of light sources to a common set of outputs.

In instances where the light source module does not include the set ofunpaired light sources 604 that is multiplexed by the first multiplexer612A, the star coupler 622 may be a 2×N star coupler with a first inputoptically connected to output 618B and a second input opticallyconnected to output 618C. It should also be appreciated that the starcoupler 622 may be replaced with any suitable wavelength-independent M×Noptical coupler.

It should be appreciated that the individual light sources of the lightsource modules described herein may be formed on one or more chips(e.g., laser dies) to form corresponding light source bars (e.g., laserbars), which may be incorporated into a photonic integrated circuit toform the light source module. The various light sources may be dividedacross different light source bars in any suitable manner. The lightsources of a given light source bar may belong to the same set or subsetof light sources discussed above, but need not. For example, in thevariation shown in FIG. 6 , light sources 602A-1 and 602A-2 of the setof unpaired light sources 604 are formed on a first light source bar620A, while light sources 602A-N-1 and 602A-N of the set of unpairedlight sources 604 are formed on a second light source bar 620B. Bothlight sources of each the first and second light source pairs (i.e.,light sources 602B-1, 602B-2, 602B-5, and 602B-6) are formed on a thirdlight source bar 620C, while both light sources of each the third andfourth light source pairs (i.e., light sources 602B-3, 602B-4, 602B-7,and 602B-8) are formed on a fourth light source bar 620D.

FIG. 7 shows another variation of a light source module 700. The lightsource module 700 is configured the same as the light source module 600of FIG. 6 (with similar components labeled the same), except that themultiplexing unit 614 has been replaced with a multiplexing unit 714. Inthis embodiment, the multiplexing unit 714 includes a set of starcouplers (including a first star coupler 702A and a second star coupler702B) and a set of switches (including a first switch 704A, a secondswitch 704B, and a third switch 704C) optically connecting themultiplexers 612A, 612B, and 612C to the set of star couplers. The firststar coupler 702A includes a first plurality of outputs 716A and thesecond star coupler 702B includes a second plurality of outputs 716B.The first plurality of outputs 716A and the second plurality of outputs716B may collectively form a set of outputs for the light source module700.

Specifically, each of the switches 704A, 704B, and 704C may beconfigured as a 1×2 controllable switch as discussed above. An input ofeach 1×2 controllable switch is connected to an output of acorresponding multiplexer of the set of multiplexers 612A, 612B, and612C, while each output of the 1×2 controllable switch is connected to adifferent star coupler of the set of star couplers 702A and 702B. Usingthe first controllable switch 704A as an example, the first controllableswitch 704A receives the output 618A of the first multiplexer 612A asits input, while the first and second outputs of the 1×2 controllableswitch are respectively optically connected to the first star coupler702A and the second star coupler 702B.

Each of the controllable switches can selectively route light receivedfrom its input entirely to its first output and thereby the first starcoupler 702A, entirely to its second output and thereby the second starcoupler 702B, or simultaneously to both the outputs and star couplers702A and 70B (i.e., split between the star couplers 702A and 702Baccording to a target splitting ratio). As a result, light generated byany light source of the light source module 700 may be selectivelyrouted to and split between one or both of the first and secondplurality of outputs 716A and 716B. Because this routing is wavelengthspecific, each controllable switch may account for the wavelength thatis currently being routed by that switch (e.g., by controlling a phasetuner of the switch as discussed above. If a given multiplexer (e.g.,the first multiplexer 612A) only receives and outputs a singlewavelength of light at a time, the adjustment of the correspondingcontrollable switch (e.g., the first controllable switch 704A) toaccount for the current wavelength allows the controllable switch to actas a wavelength-independent component.

The star couplers 702A and 702B are shown as 3×N star couplers that eachreceive a corresponding input from each of the first, second, and thirdmultiplexers 612A, 612B, and 612C via the controllable switches 704A,704B, and 704C. In instances where the light source module 700 does notinclude the set of unpaired light sources 604 and the first multiplexer612A, the star couplers 702A and 702B may optionally be configured as2×N star couplers as discussed above. As a result, light generated byany light source of the light source module 700 may be selectivelyrouted to either or both of the star couplers 702A and 70B. This lightis accordingly routed to and split between one or both of the first andsecond pluralities of outputs 716A and 716B.

During a spectroscopic measurement, one or more light sources may beactive to perform an individual measurement at a given wavelength. Insome instances, a single light source (e.g., a light source from the setof unpaired light sources 604, the first light source subset 608, or thesecond light source subset 610) may generate light at a givenwavelength, and this light may be selectively routed to one or both ofthe star couplers 702A and 702B to perform an individual measurementusing that wavelength. Conversely, when an individual measurement isperformed using a wavelength associated with a paired light source(e.g., the first pair of light sources 602B-1 and 602B-5), either ofboth of the paired light sources may be actively generating light duringa given individual measurement.

For example, light from the first light source 602B-1 and the secondlight source 602B-5 of the light source pair may simultaneously generatelight during an individual measurement that is spectroscopicallyequivalent for a given spectroscopic measurement. In some instances, thesecond and third controllable switches 704B and 704C simultaneouslyroute respective light from the first and second light sources 602B-1and 602B-5 (i.e., via the second and third multiplexers 612B and 612C)to the same selection of star couplers. For example, these switches maysimultaneously route light from the first and second light sources602B-1 and 602B-5 only to the first star coupler 702A, only to thesecond star coupler 702B, or split between the first and second starcouplers 702A and 702B. When these wavelengths are spectroscopicallyequivalent for a given spectroscopic measurement, this may increase(e.g., double) the optical power received by the star couplers 702A and702B. When these wavelengths are selected to provide different coherentnoise views, this may also reduce coherent noise associated with thespectroscopic measurement.

In other instances, the star couplers 702A and 702B may simultaneouslyreceive light from different multiplexers, which may allow the firststar coupler 702A to receive a first wavelength of light while thesecond star coupler 702B receives a second wavelength of light.Accordingly, the light source may simultaneously output the firstwavelength of light from the first plurality of outputs 716A and thesecond wavelength of light from the second plurality of outputs 716B.This may allow the optical measurement system to perform multipleindividual measurements simultaneously using two different wavelengths,with the tradeoff that each individual measurement utilizes a subset ofthe outputs of the light source module. In some of these instances, oneof the star couplers 702A and 702B also simultaneously receives light ofa third wavelength. For example, the first star coupler may receivelight generated by a light source of the set of unpaired light sources604 (e.g., light source 602A-1), and the first set of outputs 716Aoutput light of a first wavelength (λ_(A-1)). The second star coupler702B simultaneously receives light from a light source pair (e.g., lightsource 602B-1 and 602B-5), and the second set of outputs 716B outputslight with the first and second wavelengths (λ_(B-1) and λ_(B-1)+Δ₁).

While shown in FIG. 7 as having two star couplers 702A and 702B, thelight source module 700 may alternatively have a set of star couplersincluding three of more star couplers (any of which may be replaced byanother suitable optical coupler). In these instances, the light sourcemodule 700 may include wavelength-independent optical couplers and/oradditional controllable switches positioned between the multiplexers612A, 612B, and 612C and the three or more star couplers to facilitateforming an optical connection between each of the multiplexer outputs618A, 618B, and 618C and each star coupler.

FIG. 8 shows yet another variation of a light source module 800. Thelight source module 800 is configured the same as the light sourcemodule 600 of FIG. 6 (with similar components labeled the same), exceptthat the multiplexing unit 614 has been replaced with a multiplexingunit 814. In this embodiment, the multiplexing unit 814 is configured asa cascaded network of optical couplers that split light received fromany of the multiplexers 612A, 612B, and 612C between a plurality ofoutputs 816 that act as outputs for the light source module 800. Thecascade network of optical couplers includes a number of stages, eachhaving one or more optical couplers.

The number of stages, as well as the number of optical couplers in eachstage, depends at least in part on the number of inputs to the cascadenetwork of optical switches (e.g., how many multiplexer outputs arebeing combined) and the number of outputs 816. In the variation shown inFIG. 8 , the cascade network of optical switches has three inputs andeight outputs, and includes a first stage including a first opticalcoupler 802A and second optical coupler 802B, a second stage including afirst optical coupler 804A and a second optical coupler 804B, and athird stage including four optical couplers 806A-806D.

The first optical coupler 802A of the first stage is a 1×2 or 2×2optical coupler (e.g., with one of its inputs left disconnected) thatreceives the output 618A of the first multiplexer 612A as its input. Theoutputs of the first optical coupler 802A are each optically connectedto a first input of a corresponding optical coupler 804A or 804B of thesecond stage. In this way, light received by the first optical coupler802A of the first stage will be split between the optical couplers 804Aand 804B of the second stage.

The second optical coupler 802B of the first stage is a 2×2 opticalcoupler that receives the output 618B of the second multiplexer 612B asits first input and the output 618C of the third multiplexer 612B as itssecond input. The outputs of the second optical coupler 802B are eachoptically connected to a second input of a corresponding optical coupler804A or 804B of the second stage. In this way, light received by thefirst optical coupler 802A of the first stage will be split between theoptical couplers 804A and 804B of the second stage.

The optical couplers 804A and 804B of the second stage are 2×2 opticalcouplers, and split light received at either input between its twoinputs. Because each of these optical couplers 804A and 804B areoptically connected to each of the multiplexers 612A, 612B, 612C, theseoptical couplers 804A and 804B will output a portion of light generatedby any of the light sources (e.g., light sources of the set of unpairedlight sources 504 and the set of paired light sources 506).

The optical couplers 806A-806D of the third stage may be 1×2 opticalcouplers, each of which splits a corresponding output of an opticalcoupler 804A or 804B of the second stage into two different outputs. Asa result, while the second stage of optical couplers 804A and 804B hasfour outputs that would output a corresponding portion of lightgenerated by a given light source of the light source module 800, thethird stage of optical couplers 806A-806C doubles this number ofoutputs.

Each of the optical couplers may receive a range of differentwavelengths, and are thus configured to be wavelength independent.Because each optical coupler 802A and 802B of the first stage isoptically connected to a corresponding subset of the light source of thelight source module 800, these optical couplers 802A and 802B may betailored to operate with the wavelengths associated with these lightsources, while the optical couplers of subsequent stages may be tailoredto operate with the full range of wavelengths of the light source module800.

In instances where a multiplexing unit is capable of selectively routinglight between different subsets of outputs using controllable switches(such as the multiplexing unit 714 of FIG. 7 ), it may be desirable tostructure the multiplexing unit such that light generated by every lightsource of the light source module will pass through a common componentof the multiplexing unit. This may be useful in instances where thelight source module includes a wavelength locking unit for controllingthe wavelength emitted by the individual light sources, as a single tapmay be used to lock the wavelength generated by any of the light sourcesof the light source module.

When a light source module includes a wavelength locking unit, thewavelength locking unit can output a signal that is indicative of thewavelength or changes in wavelength of light received by the wavelengthlocking unit, which may be used by a controller (e.g., controller 140)to control a given light source to stabilize or otherwise adjust thewavelength of light emitted by that light source. Even for fixedwavelength lasers, the precise emission wavelength may vary slightlywith changes in temperature and/or injection current, and thus thewavelength locking unit may provide feedback to the controller to set astable wavelength output before or during a measurement. Any of thelight source modules described herein may utilize one or more wavelengthlocking units configured to provide feedback to one or more lightsources of the light source module.

FIG. 9 shows a variation of a light source module 900. The light sourcemodule 900 is configured the same as the light source module 600 of FIG.6 (with similar components labeled the same), except that themultiplexing unit 614 has been replaced with a multiplexing unit 914,and light source module 900 includes a wavelength locking unit 908.Additionally, the individual light sources of the set of unpaired lightsources 604 and the set of paired light sources 606 are not depicted. Asshown, the multiplexing unit 914 includes a 2×1 controllable switch902A, such as discussed above, that receives the outputs 618B and 618Cof the second and third multiplexers 612B and 612C as inputs. An outputof the 2×1 controllable switch 902A is optically connected to a firstinput of a 2×2 controllable switch 902B.

The 2×2 controllable switch 902B receives the output 618A of the firstmultiplexer 612A as its second input, and as a result light generated byany light source of the set of unpaired light sources 604, the firstlight source subset 608, or the second light source subset 610 will passthrough the 2×2 controllable switch 902B. The wavelength locking unit908 may be optically connected to the 2×2 controllable switch 902B toreceive a portion of light received by the 2×2 controllable switch 902B(e.g., using a tap as described above with respect to FIG. 4 ).Accordingly, the wavelength locking unit 908 may be used to providefeedback to any of the light sources of the light source module 900.

Additionally, the 2×2 controllable switch 902B is controllable toselectively route light received from one of its inputs to only one ofits outputs or split the light between its outputs. Accordingly, the 2×2controllable switch 902B may be used to selectively split light betweensome or all of the outputs of the multiplexing unit 914 (such asdescribed above with respect to FIG. 7 ). Additional optical elementsmay be used to further split these outputs and thereby provide a largernumber of outputs for the light source module 900. In the embodimentshown in FIG. 9 , the multiplexing unit further includes a set of 1×2controllable switches including a first 1×2 controllable switch 904A anda second 1×2 controllable switch 904B. Each controllable switch isconnected to a pair of 1×N star couplers.

Specifically, respective outputs of the first 1×2 controllable switch904A are connected to a first 1×N star coupler 906A having a firstplurality of outputs 916A and a second 1×N star coupler 906B having asecond plurality of outputs 916B. The first 1×2 controllable switch 904Amay selectively route light received by the 2×2 controllable switch 902Beither to the first 1×N star coupler 906A, to the second 1×N starcoupler 906B, or split between the first and second star couplers 906Aand 906B. Similarly, respective outputs of the second 1×2 controllableswitch 904B are connected to a third 1×N star coupler 906C having athird plurality of outputs 916C and a fourth 1×N star coupler 906Dhaving a second plurality of outputs 916D. The second 1×2 controllableswitch 904B may selectively route light received by the 2×2 controllableswitch 902B either to the third 1×N star coupler 906C, to the fourth 1×Nstar coupler 906D, or split between the third and fourth star couplers906C and 906D. Accordingly, the light source module 900 may be able tosplit light from a given light source between any combination ofpluralities of outputs 916A-916D.

FIG. 10 shows an example method 1000 of performing a spectroscopicmeasurement using the optical measurement systems described herein. Thespectroscopic measurement may include a series of measurements performedwhile emitting pairs of spectroscopically equivalent wavelengths, andoptionally a series of measurements performed while emitting differentwavelengths. For example, step 1002 may involve selecting (e.g., using acontroller as discussed above) a pair of wavelengths that arespectroscopically equivalent for that spectroscopic measurement. In someinstances, these wavelengths are separated by an amount sufficient toprovide different noise views as discussed above.

At step 1004, the optical measurement system performs a measurementusing the selected pair of spectroscopically equivalent wavelengths. Inthese instances, this involves simultaneously generating light at thepair of wavelengths (e.g., using two light sources of the light sourcemodules described above with respect to FIGS. 2A-9 ) and emitting thislight from the optical measurement system. Accordingly, a portion of asample being measured may be simultaneously illuminated by bothwavelengths of the pair.

This measurement may generate a set of measured signals. For example,one or more sensing elements of one or more detectors may measure lightreceived by the optical measurement system while the optical measurementsystem is emitting light at the pair of wavelengths. Each of thesesensing elements may output a measured signal representing the intensity(or another characteristic) of light received by that sensing element,and these signals may collectively form the set of measured signals forthat measurement. Individual signals in the set of measured signals maynot distinguish between how much of the signals comes from eachwavelength of the pair, and thus the optical measurement system maytreat this information as if it were generated at a single wavelength.

The measurement of step 1004 may be performed at a plurality ofdifferent spectroscopically equivalent wavelength pairs. Accordingly, atstep 1006 the method determines whether there are additional wavelengthpairs to be measured. If there are, the method returns to step 1002 toselect and perform another measurement. If all of the wavelength pairshave been measured, the method may optionally perform a series ofmeasurements using one or more additional measurements.

In the instance that all the wavelength pairs have been measured, awavelength is selected at step 1008. At step 1010, the opticalmeasurement system performs a measurement using the selected wavelength.This wavelength may be a wavelength produced by an unpaired light sourceor may be one wavelength of a spectroscopically equivalent wavelengthpair. In these instances, this involves generating light at a singlewavelength and emitting this light from the optical measurement system.It should be appreciated that instances where multiple measurements areperformed simultaneously, such as discussed above, this singlewavelength may be emitted from one launch site of the opticalmeasurement system and another wavelength or pair of wavelengths isemitted from a different launch site of the optical measurement system.This measurement may generate a set of measured signals in the samemanner as discussed with respect to step 1006. At step 1012, the methodincludes checking for additional wavelengths to be measured. If thereare additional wavelengths to be measured, another wavelength isselected at step 1008 and a subsequent measurement is performed at step1012.

The measurements performed in steps 1004 and 1010 may collectivelygenerate multiple sets of measured signals. Additionally, thesemeasurements may be done in any order (e.g., the measurements of step1004 need not be performed for every wavelength pair before performingsome or all of the measurements of step 1010). Once all of themeasurements are complete, spectroscopic information may be calculatedusing the sets of measured signals at step 1014. The optical measurementsystems may facilitate a wide range of analytical techniques as would bereadily understood by one of ordinary skill in the art, and thusindividual techniques for deriving spectroscopic information from a setof measurements taken at a plurality of different wavelengths will notbe discussed herein.

For a given wavelength of a pair of spectroscopically equivalentwavelengths, the optical measurement system may decide to use thewavelength alone or as part of a pair in different instances. Forexample, the method may include a step (not shown) that includesdetermining whether a pair of light sources that generate a selectedpair of spectroscopically equivalent wavelengths are both able tooperate according to a set of operating criteria (e.g., the light sourceis able to generate light at a target intensity). The operating criteriamay be the same set of criteria for both light sources, or the set ofoperating criteria applied to one light source may be different than theset of operating criteria applied to the second light source. If bothlight sources are determined to meet the set of operating criteria, theoptical measurement system will perform a measurement using the pair ofwavelengths. Conversely, if only one light source is determined to meetthe set of operating criteria, the optical measurement system willperform a measurement using the light source that met the set ofoperating criteria (and will thereby perform the measurement using onlyone wavelength of the wavelength pair). This may provide redundancy asdiscussed above by allowing the optical measurement system to perform agiven spectroscopic measurement even after failure of one light sourceof a given light source pair.

The foregoing description, for purposes of explanation, used specificnomenclature to provide a thorough understanding of the describedembodiments. However, it will be apparent to one skilled in the art thatthe specific details are not required in order to practice the describedembodiments. Thus, the foregoing descriptions of the specificembodiments described herein are presented for purposes of illustrationand description. They are not targeted to be exhaustive or to limit theembodiments to the precise forms disclosed. It will be apparent to oneof ordinary skill in the art that many modifications and variations arepossible in view of the above teachings.

Although the disclosed examples have been fully described with referenceto the accompanying drawings, it is to be noted that various changes andmodifications will become apparent to those skilled in the art. Suchchanges and modifications are to be understood as being included withinthe scope of the disclosed examples as defined by the appended claims.

What is claimed is:
 1. A method, comprising: emitting a first lightoutput having a first wavelength; emitting a second light output havinga second wavelength; combining the first light output and the secondlight output into a combined light output having the first wavelengthand the second wavelength; receiving a portion of the combined lightoutput at an optical detector, the portion of the combined light outputreturned from the sample; and determining spectroscopic information forthe sample from the portion of the combined light output; wherein: thefirst and second light outputs produce a coherent noise at the sample,the coherent noise having a coherent noise bandwidth; the spectroscopicinformation has a spectroscopic information bandwidth; the firstwavelength and the second wavelength are separated by an interstitialrange that is less than the spectroscopic information bandwidth; and theinterstitial range is greater than the coherent noise bandwidth.
 2. Themethod of claim 1, wherein: the sample is human skin; the first lightoutput is infrared light; the second light output is infrared light; andthe interstitial range is between one and four nanometers.
 3. The methodof claim 1, wherein: the first light output is emitted from a lightemitter; the operation of determining spectroscopic information for thesample is performed by a processing unit; and the light emitter, theoptical detector, and the processing unit are all within a housing. 4.The method of claim 1, wherein: the first light output is a firstinfrared light; and the second light output is a second infrared light.5. The method of claim 4, wherein the interstitial range is less thanfour nanometers.
 6. The method of claim 1, wherein the coherent noisebandwidth comprises a range of wavelengths within which two or morespectroscopic measurements of the sample have an r value that is greaterthan 0.5.
 7. The method of claim 6, wherein the coherent noise bandwidthis approximately one nanometer.
 8. A light source module, comprising: afirst semiconductor light source operative to emit a first wavelength oflight; a second semiconductor light source operative to emit a secondwavelength of light that is different than the first wavelength oflight; a first optical junction operative to provide a first lightoutput that includes the first and second wavelengths of light; a secondoptical junction operative to provide a second light output thatincludes the first and second wavelengths of light; and a multiplexeroperative to provide a combined light output, wherein: the firstwavelength of light provides a first coherent noise view and the secondwavelength of light provides a second coherent noise view, therebymitigating coherent noise.
 9. The light source module of claim 8,wherein: the first and second optical junctions are wavelength dependentmultiplexers; each of the first and second wavelengths of light arewithin four nanometers of each other; each of the first and secondwavelengths of light are spectroscopically equivalent to one another,thereby acting as redundant semiconductor light sources; and the firstand second semiconductor light sources are used together to provideincreased power.
 10. The light source module of claim 8, where each ofthe first and second wavelengths of light are spaced apart so that eachwavelength of light provides a different coherent noise view, therebymitigating coherent noise.
 11. The light source module of claim 8,wherein: the first optical junction is a first Mach-Zehnderinterferometer; and the second optical junction is a second Mach-Zehnderinterferometer.
 12. The light source module of claim 11, wherein: thefirst optical junction is operative to select one of the first or secondwavelengths of light to output first output light; and the secondoptical junction is operative to select one of third or fourthwavelengths of light to output second output light.
 13. The light sourcemodule of claim 8, wherein: each of the first and second wavelengths oflight is spectroscopically equivalent to each other.
 14. A light sourcemodule, comprising: a first set of semiconductor light sources operativeto emit a first set of wavelengths of light; a second set ofsemiconductor light sources operative to emit a second set ofwavelengths of light; a first wavelength independent coupler operativeto output: a first combined output derived from the first and secondsets of wavelengths of light; and a second combined output derived fromthe first and second sets of wavelengths of light; a second wavelengthindependent coupler operative to output: a third combined output derivedfrom the first and second sets of wavelengths of light; and a fourthcombined output derived from the first and second sets of wavelengths oflight; a first multiplexer operative to: receive the first combinedoutput; receive the second combined output; output a first half of thefirst combined output; and output a first half of the second combinedoutput; and a second multiplexer operative to: receive the firstcombined output; receive the second combined output; and output a secondhalf of the first combined output; and output a second half of thesecond combined output; wherein: the first, second, third, and fourthcombined outputs are derived from different combinations of the firstand second sets of wavelengths of light; the first set of wavelengths oflight provides a first set of coherent noise views; the second set ofwavelengths of light provides a second set of coherent noise views; andthe first and second sets of coherent noise views mitigate coherentnoise.
 15. The light source module of claim 14, wherein: the lightsource module comprises: a first waveguide coupled between the firstwavelength independent coupler and the first multiplexer; a secondwaveguide coupled between the first wavelength independent coupler andthe second multiplexer; a third waveguide coupled between the secondwavelength independent coupler and the first multiplexer; and a fourthwaveguide coupled between the second wavelength independent coupler andthe second multiplexer; at least two waveguides of the first, second,third, and fourth waveguides cross paths with one another; each of thefirst and second sets of wavelengths of light are within four nanometersof each other and are spectroscopically equivalent; and each of thefirst and second sets of wavelengths of light is each greater than onenanometer apart from a closest wavelength of light to provide coherentnoise mitigation.
 16. The light source module of claim 14, wherein: thefirst half of the first combined output is transmitted to a first launchregion; and the second half of the first combined output by the secondmultiplexer is transmitted to a second launch region.
 17. The lightsource module of claim 14, further comprising: a first waveguide coupledbetween the first wavelength independent coupler and the firstmultiplexer; a second waveguide coupled between the first wavelengthindependent coupler and the second multiplexer; a third waveguidecoupled between the second wavelength independent coupler and the firstmultiplexer; and a fourth waveguide coupled between the secondwavelength independent coupler and the second multiplexer, wherein noneof the first, second, third, and fourth waveguides crosses paths withone another.
 18. The light source module of claim 14, wherein the firstand second multiplexers are Echelle gratings.
 19. The light sourcemodule of claim 14, wherein: each of the first and second sets ofwavelengths of light is spectroscopically equivalent to one another. 20.The light source module of claim 14, wherein: the first wavelengthindependent coupler is a two by two multimode interferometer; and thesecond wavelength independent coupler is a two by two multimodeinterferometer.